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Observational constraints for solar-type Stellar winds

Published online by Cambridge University Press:  24 September 2020

Manuel Güdel Open the ORCID record for Manuel Güdel [Opens in a new window]
Manuel Güdel*
Affiliation:
University of Vienna, Department of Astrophysics Türkenschanzstr. 17, 1180 Vienna, Austria email: mailto:manuel.guedel@univie.ac.at
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Abstract

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Ionized winds from late-type main-sequence stars are important for stellar spin-down and therefore the evolution of stellar activity; winds blow an “astrosphere” into the interstellar medium that absorbs a large part of galactic cosmic rays; and the winds play a key role in shaping planetary environments, in particular their upper atmospheres. These issues have been well studied for the solar wind but little is known about winds escaping from other solar-type stars. Several methods have been devised to either detect winds directly or to infer the presence of such winds from features that are shaped by the winds. This paper summarizes these methods and discusses exemplary findings. There is need for more studies using multiple methods for the same stars.

Keywords

stars: winds, outflowsstars: rotationradio continuum: starsultraviolet: stars
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S354: Solar and Stellar Magnetic Fields: Origins and Manifestations , June 2019 , pp. 313 - 332
Copyright
© International Astronomical Union 2020

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